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How statement and proof provenance work

The first chip identifies the source of the statement or construction; the second identifies the source of its local proof or verification.

  • Literature-sourced: the exact statement appears in a cited source; only wording and notation differ.
  • AI-adapted: a semantically identical restatement of literature-sourced material, modulo indexing, notation, and boundary cases adopted by the library.
  • AI-generated: a genuinely novel statement formulated by AI, with no source for the claim itself.

These labels describe origin, not correctness: citations and verification chips remain separate evidence.

A 2026 weak-curvature F-theory QCD-axion ensemble constraint

Physical scope

Source-reported model-population inference for the paper's selected Tree, Skeleton, and K2 toric-threefold ensembles and its selected weak-curvature Kähler points. The SN1987A limit is an approximate astrophysical inference based on the source's supernova-emission model and one-dimensional simulations. The reported fraction is not a probability over all F-theory vacua or a deduction that F-theory describes nature.

Example

Fallon, Halverson, McAllister, and Marsh study source-selected F-theory models on toric threefold bases B3 with N=h1,1(B3), where h1,1(B3)=dim⁡CH1,1(B3) is the first Hodge number of the compact Kähler base. The source selects a weak-curvature Kähler point for each constructed model, where weak curvature means that α′ corrections are plausibly negligible, and estimates the QCD-axion mass mQCD using its stated effective-field-theory and instanton approximation. Across the Tree, Skeleton, and K2 ensembles, the paper reports that in every populated N≥8,791 bin at least 95% of its sampled models have mQCD>15 meV, above its adopted approximate SN1987A limit. The source does not provide precise model counts for each N bin, and its percentage is a sample frequency for those selected models and Kähler points, not a probability over all F-theory vacua.

The adopted SN1987A limit is an astrophysical inference: the paper uses axion-nucleon emission and the Raffelt criterion, based on one-dimensional supernova simulations of the observed neutrino burst. This is not a reported experiment measuring an F-theory model. The authors do not stabilize moduli and use a proxy visible sector without a suitable U(1), supersymmetry breaking, or fermion couplings.

Facts & Assumptions

Given: The paper's finite model ensembles, its selected weak-curvature Kähler points and QCD-axion mass approximation, and its source-specific interpretation of the SN1987A neutrino-burst constraint.

[A1]

Table I reports 14,627 Tree models with 35≤N≤2,591, 16,556 Skeleton models with 10≤N≤15,415, and 54 K2 models with 2,560≤N≤181,200. The source does not give precise per-bin counts. Its high-N bins therefore contain no Tree models. Fallon et al., Table I and Results

[A2]

The source adopts the approximate 15 meV QCD-axion mass limit from its axion-nucleon emissivity and Raffelt-criterion analysis of the SN1987A neutrino burst. The criterion is based on one-dimensional supernova simulations; it is an astrophysical inference, not a measured F-theory quantity. The paper does not independently audit the underlying supernova observations or simulations. Fallon et al., SN1987A and the QCD axion

[A3]

For each constructed model, the authors select a weak-curvature Kähler point using their stated gauge-coupling and supersymmetry-scale conditions, then estimate mQCD with their effective-field-theory procedure and a selected subset of instanton scales. Weak curvature is used to argue that α′ corrections are plausibly negligible; this is a source approximation, not a proved error bound. Fallon et al., Methodology

[A4]

The Results section and Fig. 3 report that in every populated bin with N≥8,791, at least 95% of the sampled models lie above the adopted 15 meV threshold. The paper gives no precise model count for each such bin. This is the authors' finite-sample report, not a probability statement for a larger population. Fallon et al., Results and Fig. 3

[F1]

Compact Kähler and rational Hodge polarization conventions fixes the compact Kähler convention for the source's base.

[F2]

Compact Kähler Hodge decomposition from elliptic harmonic forms identifies H1,1(B3) with the bidegree-(1,1) Hodge summand and the Dolbeault group H1(B3,ΩB31); it supplies finite-dimensionality under compact-Kähler and full-AC hypotheses.

[F3]

Type-IIB axiodilaton and elliptic-fiber dictionary adopts the geometric elliptic-fibration/F-theory dictionary. Its current statement supplies the context used here; this item does not use it as a proof of the reported ensemble frequency.

Verification

1.1A1givenalgebra

The source's Table I gives the maximum Tree value N=2,591<8,791, while the Skeleton and K2 ranges include values above the stated threshold. Thus no populated bin with N≥8,791 comes from Tree. The totals in [A1] are whole-ensemble counts and do not determine any individual high-N bin count.

1.2A2A3algebra

By [A3], the calculation uses one selected weak-curvature Kähler point per constructed model and a truncated instanton estimate. Comparing these source estimates with the approximate astrophysical inference [A2] therefore concerns those selected model points under the source's approximation, not all points in moduli space or a direct measurement of the compactification.

2.1A1A2A3A4step 1.2∎

The source reports the frequency in [A4]. Together with [A1] and the selection procedure in [A3], its scope is the finite sampled ensembles and selected Kähler points. Since the paper gives no per-bin counts, this item makes no stronger count claim; since the sample is selected and finite, the reported percentage is not a probability over all F-theory vacua. Its comparison remains conditional on the astrophysical inference [A2].

Remarks

The source reports that additional axions could strengthen the supernova constraint, but their effect depends on further model assumptions. It also leaves moduli stabilization, a suitable visible-sector U(1), supersymmetry breaking, and fermion couplings unresolved. None of these omissions is repaired by the reported 95% sample frequency.

Depends on

Dependency tree · 2 levels

Sources